Planetary Nebula Luminosity Function
The Planetary Nebula Luminosity Function is a photometric distance indicator that models the statistical distribution of luminosities of planetary nebulae in a galaxy, exploiting their characteristic bright [O III] λ5007 emission to identify a relatively invariant bright-end cutoff usable for estimating extragalactic distances.
176
Publications
11.9K
Citations
429
Authors
230
Institutions
Publications per year
2017–2026
13
Variants
Pnlf
Parents
176
Some Physical parameters of early-type stars
N. Panagia · The Astronomical Journal · 1973 · 776 citations
Natural Sciences, Astronomy, Physics +17
Barry F. Madore, Wendy L. Freedman · Publications of the Astronomical Society of the Pacific · 1991 · 438 citations · Full text
Natural Sciences, Astronomy, Physics +14
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429
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Max Planck Institute for Extraterrestrial Physics, Germany
12 publications · 823 citations
12
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11
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230

Kitt Peak National Observatory
Tucson, United States
16 h-index
29 publications
3.7K citations

Pennsylvania State University
State College, United States
14 h-index
35 publications
3.9K citations

Space Telescope Science Institute
Baltimore, United States
13 h-index
23 publications
1.6K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
12 h-index
25 publications
1.1K citations

Mount Stromlo Observatory
Canberra, Australia
11 h-index
11 publications
769 citations

U.S. National Science Foundation
Alexandria, United States
11 h-index
18 publications
2.3K citations

Astronomical Observatory of Capodimonte
Naples, Italy
11 h-index
20 publications
1.6K citations
Association of Universities for Research in Astronomy
Washington, United States
11 h-index
18 publications
2.2K citations
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ApJ · 64 publications · 4.8K citations
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22 publications · 1.2K citations
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AJ · 13 publications · 1.7K citations
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14 publications · 772 citations
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10 publications · 207 citations
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